Zobrazeno 1 - 9
of 9
pro vyhledávání: '"faculae [Sun]"'
Context: The bright regions in the solar chromosphere and temperature minimum have a good spatial correspondence with regions of intense photospheric magnetic field. Bright regions are visible in different emission lines and parts of the continuum. T
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2423::47307745b41368907f05349e04a2d7e4
http://urn.fi/urn:nbn:fi-fe2022102763381
http://urn.fi/urn:nbn:fi-fe2022102763381
Publikováno v:
Astronomy & Astrophysics
Vortex-flows exist across a broad range of spatial and temporal scales in the solar atmosphere. Small-scale vortices have been proposed to play an important role in energy transport in the solar atmosphere. However, their physical properties remain p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6e657a772e2fc5179f32f610729b43b2
http://arxiv.org/abs/2010.14971
http://arxiv.org/abs/2010.14971
Autor:
Giuseppina Micela, S. H. Saar, Ronald L. Walsworth, Rosario Cosentino, Annelies Mortier, David F. Phillips, A. Collier Cameron, Xavier Dumusque, Suzanne Aigrain, David W. Latham, Samantha Thompson, E. J. W. de Mooij, Raphaëlle D. Haywood, Ennio Poretti, T. W. Milbourne, Alessandro Sozzetti, M. López-Morales, Heather M. Cegla, Adriano Ghedina, David Charbonneau, A. Thompson, Emilio Molinari, J. Costes, Christopher A. Watson
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Thompson, A P G, Watson, C A, Haywood, R D, Costes, J C, de Mooij, E, Collier Cameron, A, Dumusque, X, Phillips, D F, Saar, S H, Mortier, A, Milbourne, T W, Aigrain, S, Cegla, H M, Charbonneau, D, Cosentino, R, Ghedina, A, Latham, D W, López-Morales, M, Micela, G, Molinari, E, Poretti, E, Sozzetti, A, Thompson, S & Walsworth, R 2020, ' The spectral impact of magnetic activity on disc-integrated HARPS-N solar observations: exploring new activity indicators ', Monthly Notices of the Royal Astronomical Society, vol. 494, no. 3, pp. 4279-4290 . https://doi.org/10.1093/mnras/staa1010
Thompson, A P G, Watson, C A, Haywood, R D, Costes, J C, de Mooij, E, Collier Cameron, A, Dumusque, X, Phillips, D F, Saar, S H, Mortier, A, Milbourne, T W, Aigrain, S, Cegla, H M, Charbonneau, D, Cosentino, R, Ghedina, A, Latham, D W, López-Morales, M, Micela, G, Molinari, E, Poretti, E, Sozzetti, A, Thompson, S & Walsworth, R 2020, ' The spectral impact of magnetic activity on disc-integrated HARPS-N solar observations: exploring new activity indicators ', Monthly Notices of the Royal Astronomical Society, vol. 494, no. 3, pp. 4279-4290 . https://doi.org/10.1093/mnras/staa1010
Stellar activity is the major roadblock on the path to finding true Earth-analogue planets with the Doppler technique. Thus, identifying new indicators that better trace magnetic activity (i.e. faculae and spots) is crucial to aid in disentangling th
Publikováno v:
Astronomy and Astrophysics
We study the properties of slow magneto-acoustic waves that are naturally excited due to turbulent convection and investigate their role in the energy balance of a plage region using three dimensional (3D) radiation-MHD simulations. We calculate the
Autor:
Giuseppina Micela, Rosario Cosentino, D. W. Latham, Adriano Ghedina, Heather M. Cegla, David F. Phillips, D. Charbonneau, Samantha Thompson, Steven H. Saar, Timothy Milbourne, C. H. Li, M. Lopez-Morales, Alessandro Sozzetti, C. Lovis, Andrew Szentgyorgyi, François Bouchy, Christopher A. Watson, M. Gonzalez, Stéphane Udry, Emilio Molinari, M. L. Palumbo, N. Buchschacher, Andrew Collier Cameron, Ken Rice, Jesus Maldonado, J. Costes, Francesco Pepe, Alex Glenday, Massimo Cecconi, L. Malavolta, Xavier Dumusque, Raphaëlle D. Haywood, D. Segransan, G. Piotto, M. Mayor, Annelies Mortier, Dimitar Sasselov, Nicholas Langellier, Ronald L. Walsworth, Marcello Lodi
Publikováno v:
BASE-Bielefeld Academic Search Engine
Milbourne, T W, Haywood, R D, Phillips, D F, Saar, S H, Cegla, H M, Cameron, A C, Costes, J, Dumusque, X, Langellier, N, Latham, D W, Maldonado, J, Malavolta, L, Mortier, A, Palumbo, M L III, Thompson, S, Watson, C A, Bouchy, F, Buchschacher, N, Cecconi, M, Charbonneau, D, Cosentino, R, Ghedina, A, Glenday, A G, Gonzalez, M, Li, C-H, Lodi, M, López-Morales, M, Lovis, C, Mayor, M, Micela, G, Molinari, E, Pepe, F, Piotto, G, Rice, K, Sasselov, D, Ségransan, D, Sozzetti, A, Szentgyorgyi, A, Udry, S & Walsworth, R L 2019, ' HARPS-N Solar RVs Are Dominated by Large, Bright Magnetic Regions ', The Astrophysical Journal, vol. 874, no. 1 . https://doi.org/10.3847/1538-4357/ab064a
Milbourne, T W, Haywood, R D, Phillips, D F, Saar, S H, Cegla, H M, Cameron, A C, Costes, J, Dumusque, X, Langellier, N, Latham, D W, Maldonado, J, Malavolta, L, Mortier, A, Palumbo, M L III, Thompson, S, Watson, C A, Bouchy, F, Buchschacher, N, Cecconi, M, Charbonneau, D, Cosentino, R, Ghedina, A, Glenday, A G, Gonzalez, M, Li, C-H, Lodi, M, López-Morales, M, Lovis, C, Mayor, M, Micela, G, Molinari, E, Pepe, F, Piotto, G, Rice, K, Sasselov, D, Ségransan, D, Sozzetti, A, Szentgyorgyi, A, Udry, S & Walsworth, R L 2019, ' HARPS-N Solar RVs Are Dominated by Large, Bright Magnetic Regions ', The Astrophysical Journal, vol. 874, no. 1 . https://doi.org/10.3847/1538-4357/ab064a
State-of-the-art radial-velocity (RV) exoplanet searches are currently limited by RV signals arising from stellar magnetic activity. We analyze solar observations acquired over a 3 yr period during the decline of Carrington Cycle 24 to test models of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9121ce527c2b3f924dcbafc9c92a0a8d
https://hdl.handle.net/10023/17411
https://hdl.handle.net/10023/17411
Context.Changes in solar irradiance and in its spectral distribution are among the main natural drivers of the climate on Earth. However, irradiance measurements are only available for less than four decades, while assessment of solar influence on Ea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e60abaf744abf2afa094ae31ffac8638
http://arxiv.org/abs/1811.03464
http://arxiv.org/abs/1811.03464
Publikováno v:
Astronomy & Astrophysics. Elsevier
Astronomy & Astrophysics
Astronomy & Astrophysics
We present observations testing the Dopplergram capability of a narrow-band (80 mÅ) Lyot filter imaging the solar surface in the wings of the Ba II 4554 Å resonance line in combination with speckle reconstruction to obtain high angular resolution.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::81ad4b2bcc9b1e99664e71e5b192426f
https://dspace.library.uu.nl/handle/1874/1177
https://dspace.library.uu.nl/handle/1874/1177
Autor:
Dan Kiselman, Vasco M. J. Henriques
Publikováno v:
Astronomy & Astrophysics. 557:A5
Aims. We aim at gaining insight into the thermal properties of different small-scale structures related to sunspots. Methods. We use filtergrams in the Ca II H filter at the Swedish 1-m Solar Telescope to study the relationship between fine structure
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